The evolution of galaxies is governed mainly by the evolution of massive stars whereas the evolution of a massive star depends primarily on its mass, chemical composition and on whether or not the star is a Single object or a binary component. To study the evolution of galaxies, it is therefore essential to know how stellar masses are distributed at birth, how many stars are formed in binaries, and what the mass ratio and orbital period distribution of binaries look like. Massive stars are intrinsically the brightest stars, so that it may be possible to discover their properties in distant groups prOvided that large telescopes can be used for basic stellar observations. However, until now the observations of massive stars have been reasonably complete only for a small region of our own Galaxy (~ 3 kpc from the Sun). One hopes that the conclusions resulting from these observations hold for the whole Galaxy, for the whole cosmos. With 'The Brightest Stars' of De Jager (1980) in mind, the present monograph is an addendum and an update in which we discuss the observations of 'The Brightest Binaries' in the framework of stellar evolution. A small or intermediate mass star close to the Sun may look brighter than a massive one far away. However, within volume limited star samples, the massive stars are on average also the brightest ones. In the present monograph (similarly as in the work of De Jager), bright means massive. The book consists of four main chapters.
Le informazioni nella sezione "Riassunto" possono far riferimento a edizioni diverse di questo titolo.
Introduction. List of Abbreviations. Constants. I. Massive Stars. II. Massive Single Stars. III. Massive Close Binaries. IV. Massive Star Population Number Synthesis. Concluding Remarks. References. Index.
Le informazioni nella sezione "Su questo libro" possono far riferimento a edizioni diverse di questo titolo.
Da: Lucky's Textbooks, Dallas, TX, U.S.A.
Condizione: New. Codice articolo ABLIING23Mar2411530140975
Quantità: Più di 20 disponibili
Da: Ria Christie Collections, Uxbridge, Regno Unito
Condizione: New. In. Codice articolo ria9781402003769_new
Quantità: Più di 20 disponibili
Da: Books Puddle, New York, NY, U.S.A.
Condizione: New. pp. 356. Codice articolo 2647971694
Quantità: 4 disponibili
Da: Kennys Bookshop and Art Galleries Ltd., Galway, GY, Irlanda
Condizione: New. Series: Astrophysics and Space Science Library. Num Pages: 356 pages, biography. BIC Classification: PHVB. Category: (G) General (US: Trade). Dimension: 235 x 155 x 18. Weight in Grams: 545. . 2001. Softcover reprint of the original 1st ed. 1998. Paperback. . . . . Codice articolo V9781402003769
Quantità: 15 disponibili
Da: THE SAINT BOOKSTORE, Southport, Regno Unito
Paperback / softback. Condizione: New. This item is printed on demand. New copy - Usually dispatched within 5-9 working days 530. Codice articolo C9781402003769
Quantità: Più di 20 disponibili
Da: Majestic Books, Hounslow, Regno Unito
Condizione: New. Print on Demand pp. 356 49:B&W 6.14 x 9.21 in or 234 x 156 mm (Royal 8vo) Perfect Bound on White w/Gloss Lam. Codice articolo 44843697
Quantità: 4 disponibili
Da: Biblios, Frankfurt am main, HESSE, Germania
Condizione: New. PRINT ON DEMAND pp. 356. Codice articolo 1847971684
Quantità: 4 disponibili
Da: Revaluation Books, Exeter, Regno Unito
Paperback. Condizione: Brand New. 1st edition. 356 pages. 9.24x0.74x6.26 inches. In Stock. Codice articolo x-1402003765
Quantità: 2 disponibili
Da: Kennys Bookstore, Olney, MD, U.S.A.
Condizione: New. Series: Astrophysics and Space Science Library. Num Pages: 356 pages, biography. BIC Classification: PHVB. Category: (G) General (US: Trade). Dimension: 235 x 155 x 18. Weight in Grams: 545. . 2001. Softcover reprint of the original 1st ed. 1998. Paperback. . . . . Books ship from the US and Ireland. Codice articolo V9781402003769
Quantità: 15 disponibili
Da: moluna, Greven, Germania
Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. The evolution of galaxies is governed mainly by the evolution of massive stars whereas the evolution of a massive star depends primarily on its mass, chemical composition and on whether or not the star is a Single object or a binary component. To study the . Codice articolo 4091799
Quantità: Più di 20 disponibili